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Fig. 1.
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Relationship between the X-ray luminosity LX and optical-UV luminosity LUV in RLAGNs with an EUV deficit, where the blue line represents our best-fitting result. The green line is the best-fitting result for RQAGNs given by Lusso et al. (2010). The red line corresponds to the relationship for RLAGNs without an EUV deficit.
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